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Lithos

Volume 75, Issues 1–2, July 2004, Pages 115-139
Lithos

Amphibole genesis via metasomatic reaction with clinopyroxene in mantle xenoliths from Victoria Land, Antarctica

https://doi.org/10.1016/j.lithos.2003.12.021Get rights and content

Abstract

Petrographic and major and trace element geochemical features of clinopyroxene, amphibole and glass from composite xenoliths from Mt. Melbourne and Mt. Overlord (Victoria Land, Antarctica) were investigated. Amphibole disseminated in the peridotite matrix appears to grow around clinopyroxene and spinel, and is often associated with high-TiO2 silicate glass. Clinopyroxene presents a wide range of compositions, from primary unmetasomatized diopside to high-MgO salite, with REE patterns varying from flat (at YbN 5Xchondrite) to slightly enriched [(La/Yb)N 2.7–4.2] at higher HREE contents (YbN 9.3–14.3). Amphibole also occurs in veins which, in few cases, grade into glass-rich veins before vanishing into the peridotite. Glasses are not related to amphibole destabilization; on the contrary, they appear to be strictly related to its formation. No chemical differences were noted between glasses related to disseminated or vein amphiboles. Their geochemical features favour a Na-alkaline silicate melt as the metasomatizing agent. Mass balance calculations were used to model the reactions producing amphibole from primary clinopyroxene, and to highlight the nature of the metasomatic agent/s. Trace element contents of the inferred melt/s are comparable to those of the most undersaturated magma found in the area, suggesting a strong link between metasomatism and the magmatism of the Ross Sea Rift system. This hypothesis is further strengthened by the analogy between trace element patterns of clinopyroxene associated with amphibole (cpx-A) and those of clinopyroxene contaminated by the host basalt (cpxBas). On the basis of the Mg/Fe diffusion model, the difference in mg# between these two clinopyroxenes was used to estimate the timing of the basalt infiltration and amphibole formation. Finally, various models for disseminated and vein amphibole relationships are recalled and their application to Antarctic amphiboles is tested. The petrographic and geochemical features of disseminated amphiboles, in fact, do not support the hypothesis that they may derive from differentiated magma after vein amphiboles have crystallized. Both amphibole types may have formed within a similar time span due to the different magma/wall rock ratios which control the mode of melt migration from porous flow to cracking and fracturing.

Introduction

Mantle xenoliths from Mt. Melbourne and Mt. Overlord (Victoria Land, Antarctica) occur in scoria cones and in basanitic to tephritic lavas. Alkaline to tholeiitic magmatism in this area started in the early Eocene in relation to the Ross Sea Rift system, which is situated along the eastern border of the Transantarctic mountains Fitzgerald et al., 1987, Beccaluva et al., 1991a. The rift system is organized in two main branches: one inland, trending NNW–SSE up to Mt. Overlord, while the other, toward the sea, is directed NE–SW. Petrological features and thermobarometric evolution of the lithospheric mantle from Cape Washington to Mt. Overlord were discussed in Beccaluva et al. (1991b), and more recently by Perinelli and Armienti (2002). However, several peculiar petrographic and geochemical features related to the widespread presence of amphibole remain untreated. In particular, the occurrence (and the strict association in several xenoliths) of amphibole, clinopyroxene and glasses provides a unique opportunity for investigating amphibole formation in relation to metasomatism, eventually leading to the hydration of anhydrous mantle.

It is well-known that amphibole represents a key mineral in mantle paragenesis as it is one of the main hosts for alkalis. Its role is crucial in basalt petrogenesis even at high degrees of partial melting (Beccaluva et al., 1998), as well as in mantle glass genesis via decompression or in situ melting processes Chazot et al., 1996a, Yaxley and Kamenetsky, 1999, Yaxley et al., 1997.

Disseminated amphibole growing around clinopyroxene and/or spinel is commonly observed Francis, 1976, Fabriés et al., 1987, Vaselli et al., 1996, Gregoire et al., 1997, Dawson and Smith, 1988, Bodinier et al., 1990, Zanetti et al., 1996, Woodland et al., 1996, Moine et al., 2001, Ionov et al., 2002, though its genesis is often referred to previous, generally poorly defined, metasomatic event/s Zanetti et al., 1996, Witt-Eickschen et al., 1998. Zanetti et al. (1996) distinguish two kinds of disseminated amphiboles: one older, produced by a previous metasomatism, and one younger, occurring only in the proximity of amphibole veins, related to the infiltration into the wall-rock by the same liquid generating the veins. On the other hand, vein amphiboles are usually considered products of direct crystallization from basanite or alkali basalt magmas in the upper mantle Francis, 1976, O'Reilly, 1987, O'Reilly et al., 1991, Dawson and Smith, 1988, Ionov et al., 1997, Witt-Eickschen et al., 1998, Moine et al., 2001. The residual melt afterward infiltrates the peridotite matrix, creating new amphibole in the form of crystallization or reaction products.

Some inconsistency arises in those models where disseminated amphiboles are (i) older and separated from the magmatic event which created the vein amphibole, even if chemical composition may be quite comparable and, in any case, leaving the petrogenesis of disseminated amphibole unsolved; or (ii) younger and formed by differentiated melts, even if major element contents (especially mg#) are very similar, and melt propagating through fracturing precedes porous flow migration. Thus, notwithstanding the large amount of papers reported above, the chemical and temporal relationships between disseminated and vein amphibole is still a matter of considerable debate. Moreover, to the best of the authors' knowledge, glasses related to amphibole formation have not been reported. Most studies regarding amphibole genesis were, in fact, developed on alpine peridotite massifs Woodland et al., 1996, McPherson et al., 1996, Zanetti et al., 1996 where glass cannot be preserved, or else in mantle xenoliths where amphibole and glass were related to either decompressional (Laurora et al., 2001) or in situ melting Chazot et al., 1996a, Yaxley and Kamenetsky, 1999 of volatile-bearing phases; in both cases amphibole is consumed, and glass plus secondary phases are produced.

As it will be shown below, amphibole in lithospheric mantle from Antarctica is growing at the expense of clinopyroxene and is always associated with glass, thus offering a unique opportunity to study the genetic processes (and metasomatic agent/s) responsible for its formation. To this purpose a painstaking petrographic study was accompanied by a major and trace element microanalytical work mainly addressing clinopyroxene, amphibole (disseminated in the peridotite matrix and in the vein) and glass compositional variations. The effects of host basalt infiltration were also studied in order to isolate host basalt contamination from metasomatic processes. Finally, a comparison between petrological features of the inferred metasomatic agent/s, and the basalts of the Ross Sea Rift system is presented, setting metasomatism and magmatism within a unique framework.

Of particular interest is the paper of Gamble and Kyle (1987), who studied an amphibole-glass-bearing wehrlite from Foster Crater (Antarctica) with textural features identical to those observed in the Mt. Melbourne peridotites; their data and model for amphibole, glass and host magma relationships were, in our opinion, really outstanding for the time. Our investigations however include also lherzolites, thus extending the study to more “common” mantle parageneses. Moreover, the interpretation of Gamble and Kyle (1987) of glasses as simple differentiation products from magmas similar to the host basalts after amphibole crystallization does not agree with our study.

Samples were collected during the Italian Antarctic expedition in the late 1980s. Numbers refer to localities, while letters indicate different xenoliths. Amphibole-bearing peridotites occur mainly in one locality north of Mt. Melbourne and, subordinately, in another west of Mt. Overlord. The studied samples represent all the amphibole-bearing xenoliths found (see also Beccaluva et al., 1991b for further description).

Section snippets

Petrography

The Antarctic xenoliths consist of both anhydrous and hydrous (mainly amphibole-bearing) lherzolites. Protogranular is the most common primary texture on which several types of secondary pyrometamorphic (metasomatic) textures are superimposed Mercier and Nicolas, 1975, Pike and Schwartzam, 1977. Hydrous peridotites are characterized by disseminated amphiboles in the peridotite matrix, and in veins: the former are always associated with spinel (Fig. 1A,C) and clinopyroxene (Fig. 1B,D), sometimes

Analytical methods

Major element analyses of minerals and glasses were carried out on a Cameca SX100 electron microprobe at the Institute of Petrology, Vienna University, the operating conditions were 15 kV and 20 nA. In order to reduce alkali loss, glass analyses were performed using a defocused beam with a diameter of 5–10 μm at 15kV and 10nA. The error for all elements is below 5%, except for Na, which may be up to 10%. Natural and synthetic standards were used for calibration, and the PAP correction (Pouchou

Phase geochemistry

The following description will be mainly focussed on compositional variations of clinopyroxene, amphibole and glass, thus neglecting olivine and spinel, whose variations in relation to metasomatism have already been discussed by several authors (Bonadiman et al., 2001, and references therein). As is usually observed for anhydrous parageneses, secondary olivine tends to be higher in mg# [Mg/(Mg+FeT) at.%] and spinel higher in cr# [Cr/(Cr+Al) at.%] compared to their primary counterparts.

Metasomatic melt/s and relationships with the Ross Sea magmatic system

The reactions which eventually lead to amphibole formation are modelled by mass balance calculations, which also made it possible to highlight the chemical characteristics of the metasomatic agents. The mass balance model is based on major element composition of primary and secondary minerals, with the metasomatic melt as the unknown. Reaction coefficients, obtained assuming a least-squares residue always <1.0 (Table 4), were then used for trace element calculations combined with the reactive

Evolutionary model

The distinction between contamination by the host basalt during (or shortly before) the uprising and metasomatism, i.e. infiltration of magmas at mantle level, is not at all straightforward, particularly when the metasomatic melt has comparable geochemical features to the host basalt, and could hence be considered as part of a continuous process ultimately leading to magma formation. In order to present the evolutionary model starting from metasomatic enrichment through amphibole formation up

Disseminated and vein amphiboles

As reported in the Phase geochemistry section, disseminated and vein amphiboles have similar major and trace element compositions (Fig. 4), which is a peculiar feature of Antarctic amphiboles.

Most of the disseminated and vein amphiboles reported in literature, in fact, show remarkable differences both in major and trace element distribution between the two types Dawson and Smith, 1988, Ionov et al., 1997, Moine et al., 2001.

In amphibole-bearing peridotites, amph-D growing around and in reaction

Conclusions

The petrographic and geochemical features of composite amphibole-bearing xenoliths from Antarctica indicate that amphibole is formed by reaction between the metasomatic melt and primary anhydrous parageneses, mainly at the expense of clinopyroxene and spinel. Clinopyroxene is the mineral that records the widest compositional variation during this reaction, and was probably pre-LREE-enriched through diffusion processes. It increases its TiO2, Al2O3 and HREE contents when the melt comes into

Acknowledgments

The authors are indebted to S. O'Reilly, G. Yaxley and A. Woodland for their constructive reviews. Woodland in particular made a series of pertinent comments, which allowed us to better constrain the first draft of the reaction model.

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